Gravitational Radiation from Post-Newtonian Sources and Inspiralling Compact Binaries
Author:
Publisher
Springer Science and Business Media LLC
Subject
Physics and Astronomy (miscellaneous)
Link
http://link.springer.com/content/pdf/10.12942/lrr-2014-2
Reference428 articles.
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3. Ajith, P., Iyer, B. R., Robinson, C. A. K. and Sathyaprakash, B. S., “New class of post-Newtonian approximants to the waveform templates of inspiralling compact binaries: Test mass in the Schwarzschild spacetime”, Phys. Rev. D, 71, 044029 (2005). [gr-qc/0412033]. (Cited on pages 65 and 131.)
4. Ajith, P. et al., “Template bank for gravitational waveforms from coalescing binary black holes: Nonspinning binaries”, Phys. Rev. D, 77, 104017 (2008). [DOI], [ADS], [arXiv:0710.2335 [gr-qc]]. Erratum: Phys. Rev. D, 79, 129901(E) (2009). (Cited on page 65.)
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